Showing posts with label galaxy. Show all posts
Showing posts with label galaxy. Show all posts

Wednesday, February 26, 2014

Chasing the Gaia Glint

IMAGE CREDIT: Dr Scott Ferguson Capture the Gaia tilt back (8th March) from T31 at Q62 Siding Spring, NSW, Australia.

UPDATE: 8th Mar: Gaia glints again. Today the Gaia mission controllers tilted the spacecraft again from 45 degrees to 42 degrees then 0 degrees and back again. It was tilted more slowly this time to allow astronomers to get a more detailed light curve of the tilt. Mission controllers are problem solving a stray light issue that was picked up during commissioning tests.

UPDATE:28th Feb: Patrick Wiggins animated gif of Gaia.

Image Credit: (C) Patrick Wiggins

UPDATE 27th Feb: I missed it on both 26th and 27th due to cloud. However Scott Ferguson captured one image of it on 27th before also losing out to cloud. Patrick Wiggins has captured it and had it verified by other notables on the Minor Planet List.

Image Credit: Dr Scott Ferguson 2014-Feb-27 08:52 09h 50m 24.95s, +17d 32' 30.5" 8:52 UT from Observatory H06. Note the above plot is for Modesto California so the position is a lttile off in the map. The JPL Ephemeris tool for the LAT/Long of H06 was for 2014-Feb-27 09:00 09 50 24.95 +17 32 21.8 which is just a couple of arcsecs off. Given he only had one image, Scott also verified the position with a previous Mt Palomar plate of the location.

Image Credit: ESA GBOT (ground based observation tools) FOV output for the 2nd tilt on 27th Feb developed by S. Bouquillon & T. Carlucci utilizing Stilts , Aladin , ESO online digitized Sky Survey , CDSclient.

Amateur astronomers tonight are chasing the Gaia Glint.

As the Gaia spacecraft rounds the L2 Lagrange Point tonight on its mission to create a 3d map of our solar system, around 10:45 Local time [11:45 UT] the solar panels will turn back around to "flash" earth for about 24 hours.

Sadly the weather is looking poor at two of iTelescope.net's sites.

The ESA mission controllers have asked for a light curve of the turn. Easy peasy .... or so it seems.

The targeting is not the issue, the spacecraft will cruise in at Mag 20 to 20.5 and then over a period of 15-20 minutes will brighten to magnitude 15. Whilst magnitude 15 is within reach of most amateurs with sophisticated goto scopes, Mag 20.5 is a different prospect, requiring probably a few stacked images as it brightens. So its going to be hard to make it look any different to "off" & "on" and trap the subtelties of the rising magnitude.

Never one to shirk a challenge we'll give it a go. If not we can have another go tomorrow night as the spacecraft turns again and the reverse happens (fades from Mag 15 to 20).

I'm sure someone will catch it, there are a couple of others I know who are chasing it.

The spacecraft is going through some very detailed and precise commissioning tests as it orbits the L2 Lagrange point. When fully operational the spacecraft is required to maintain a constant spin rate of 0.016656 degrees per second, which is one rotation every 6 hours & 14.23 seconds. One of the comissioning tests was to put the spacecraft through a tilt from 0 to 45 degrees and back again, and like all good scientists they wanted an independent source of data to confirm the tilt process was completed properly and smoothly, and confirmed by their on board instruments as well as visually. Amateur astronomers are always up for a challenge and like to assist and be involved in the mission.

Wednesday, January 8, 2014

Black Eye in the Sky!

Today's image in my Southern Summer/ Northern Winter image series highlighting some of the seasonal delights for astronomers is M64, commonly known as the "Black Eye" Galaxy.

Its a deep sky object, as its quite small in size but quite bright none the less. The so called "Black Eye" is caused by thick dust lanes of the spiral galaxy blocking some of the central star light. The darker thick dust lanes being on the closer side from our perspective.

It often reminds me of looking over a thick eye-wall of a hurricane.

The M64 is its number in the Messier Catalogue, a list of "fuzzy objects" compiled by Charles Messier in the 1700's that were known to be not comets.

So over the course of January, I'll be posting daily images some of these highlights of the night sky. Today's image was taken last night from New Mexico H06 on 0.5m Planewave, a 300 sec exposure with the Luminance filter.

Enjoy!

Monday, July 4, 2011

Blondes in Space!


Image: The APEX Telescope, Chajnantor, Chile. Credit: J. Vieira/APEX (MPIfR/ESO/OSO)

I am going to have so much fun with this, and as a blogger, my role is to make the science "fun and engaging" for a whole new generation of non-sciency people!

I could have gone with any of:-

Blondes in Space!
Hair Salon at the end of the universe!
So long and thanks for all the perms!
The hairdresser's guide to the galaxy!

Photo Credit: Newfreephotos.com

Ah.....where do I start.

Reece Witherspoon in Legally Blonde, showed us how important it was, - you can win lawsuits with a good knowledge of haircare products.

Australian cricketers know they are about to loose the Ashes when the English cricketers start spending more money on hydrogen peroxide - yes those blonde tips. There is a mathematical relationship between confidence and expenditure on hydrogen peroxide.

However, life on this planet depends not just on a good stylist, hydrogen peroxide also plays a key role in the chemistry of water and ozone in our planet’s atmosphere. Ozone protects us from harmful radiation, but can fluctuate in our upper atmosphere and this chemistry is widely studied here on earth. So want about Space - is it out there?

Submillimetre astronomy is a relatively unexplored frontier in astronomy and reveals a Universe that cannot be seen in the more familiar visible or infrared light. It is ideal for studying the "cold Universe": light at these wavelengths shines from vast cold clouds in interstellar space, at temperatures only a few tens of degrees above absolute zero.

The European Southern Observatory (ESO) today announced
that astronomers had detected Hydrogen Peroxide - H2O2 in a gas cloud in our own galaxy, near the naked eye star, Rho Ophiuchi in Ophiuchus. This is a beautiful area of the night sky instantly recognizable by keen astro-photographers.


Image Credit: ESO/S. Guisard (www.eso.org/~sguisard)

How did they do that - flux capacitor hooked up to a hair dryer?

An international team of astronomers made the discovery with the Atacama Pathfinder Experiment telescope (APEX), situated on the 5000-metre-high Chajnantor plateau in the Chilean Andes. They observed a region in our galaxy close to the star Rho Ophiuchi, about 400 light-years away. The region contains very cold (around -250 degrees Celsius), dense clouds of cosmic gas and dust, in which new stars are being born. The clouds are mostly made of hydrogen, but contain traces of other chemicals, and are prime targets for astronomers hunting for molecules in space. Telescopes such as APEX, which make observations of light at millimetre- and submillimetre-wavelengths, are ideal for detecting the signals from these molecules.

Image Credits: ESO, IAU and Sky & Telescope

Now that is one serious telescope, APEX is a collaboration between the Max-Planck Institute for Radio Astronomy (MPIfR), the Onsala Space Observatory (OSO) and operated by ESO.

We were really excited to discover the signatures of hydrogen peroxide with APEX. We knew from laboratory experiments which wavelengths to look for, but the amount of hydrogen peroxide in the cloud is just one molecule for every ten billion hydrogen molecules, so the detection required very careful observations,” says Per Bergman, astronomer at Onsala Space Observatory in Sweden. Bergman is lead author of the study, which is published in the journal Astronomy & Astrophysics.

ESO, the European Southern Observatory, is the foremost intergovernmental astronomy organisation in Europe and the world’s most productive astronomical observatory. It is supported by 15 countries: Austria, Belgium, Brazil, the Czech Republic, Denmark, France, Finland, Germany, Italy, the Netherlands, Portugal, Spain, Sweden, Switzerland and the United Kingdom. ESO carries out an ambitious programme focused on the design, construction and operation of powerful ground-based observing facilities enabling astronomers to make important scientific discoveries.

Hydrogen peroxide is thought to form in space on the surfaces of cosmic dust grains — very fine particles similar to sand and soot — when hydrogen (H) is added to oxygen molecules (O2). A further reaction of the hydrogen peroxide with more hydrogen is one way to produce water (H2O). This new detection of hydrogen peroxide will therefore help astronomers better understand the formation of water in the Universe.

So why all the fuss you ask?

We don’t understand yet how some of the most important molecules here on Earth are made in space. But our discovery of hydrogen peroxide with APEX seems to be showing us that cosmic dust is the missing ingredient in the process,” says Bérengère Parise, head of the Emmy Noether research group on star formation and astrochemistry at the Max-Planck Institute for Radio Astronomy in Germany, and a co-author of the paper.

The new discovery of hydrogen peroxide may also help astronomers understand another interstellar mystery: why oxygen molecules are so hard to find in space. It was only in 2007 that oxygen molecules were first discovered in space, by the satellite Odin.

Congratulations to the international team on another great, exciting discovery, using the ESO/APEX telescope at Chajnantor.

So I'll sign off with - do Astronomer's really have more fun? Absolutely!

Saturday, June 13, 2009

M104 Sombrero Galaxy


The amazing M104 Sombrero Galaxy. Not sure which is the most amazing aspect, the Galaxy itself, the amazing surrounding sky, or the fact that Vesto Slipher calculated in 1912 that it is traveling away from us at 1000 klms per second.

This 60 mins HA (3nm) shot taken by the author with ASA N16 16" Astrograph with FLI PL11002 class 1.

High res version

www.aartscope.com

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